搜索

x

留言板

尊敬的读者、作者、审稿人, 关于本刊的投稿、审稿、编辑和出版的任何问题, 您可以本页添加留言。我们将尽快给您答复。谢谢您的支持!

姓名
邮箱
手机号码
标题
留言内容
验证码

大尺度分层介质电特性参数的反演方法研究

张宇 张晓娟 方广有

引用本文:
Citation:

大尺度分层介质电特性参数的反演方法研究

张宇, 张晓娟, 方广有

A data inversion method for electromagnetic scattering from large-scale layered medium

Zhang Yu, Zhang Xiao-Juan, Fang Guang-You
PDF
导出引用
  • 针对大尺度分层介质电磁场散射回波数据, 提出了一种用于分层介质特性参数反演的新方法, 实现了分层介质的介电常数、电导率和介质厚度的同时反演. 方法首先将这些参数的反演转化为最优化问题进行求解, 然后应用模拟退火算法搜索最优解, 充分利用算法的全局寻优能力, 同时改善了算法的搜索控制策略, 使算法在最优解的搜索过程中可以自适应地调整搜索步长, 提高了算法的搜索效率. 结果表明, 本文方法可以实现大尺度分层介质特性参数的准确反演, 且具有较强的抗噪声能力. 该方法可以应用于火星/月球 雷达探测回波数据的反演以及地下分层结构特性的分析.
    An inversion method for electromagnetic scattering echo data from large-scale layered medium is presented to simultaneously retrieve the electromagnetic property parameters of the medium. Firstly, the inversion is converted into an optimization problem. Then the simulating annealing algorithm is adopted to find the optimal solution by taking full advantage of the algorithm global optimization. Besides, the search control strategy of the algorithm is optimized so that the algorithm can adaptively adjust the search step in the optimal solution search process. The search efficiency of the algorithm is improved by these optimizations. Results show that the proposed method can achieve an accurate result in the inversion of the characteristic parameters of large-scale layered media as well as a strong anti-noise ability. The inversion method presented can be applied to the Mars/lunar radar echo data inversion and analysis of underground layered medium.
    • 基金项目: 国家自然科学基金(批准号:61172017,60890071-01)资助的课题.
    • Funds: Project supported by the National Natural Science Foundation of China (Grant Nos. 61172017, 60890071-01).
    [1]

    Ilyushin Y A 2007 Planet. Space Sci. 55 100

    [2]

    Kobayashi T, Oya H, Ono T 2002 Earth Planets Space 54 973

    [3]

    Spagnuolo M G, Grings F, Perna P, Franco M, Karszenbaun H, Ramos V A 2011 Planet. Space Sci. 59 1222

    [4]

    Zhang Y Q, Ge D B 2009 Acta Phys. Sin. 58 4573 (in Chinese) [张玉强, 葛德彪 2009物理学报 58 4573]

    [5]

    Guo L X, Wang Y H, Wu Z S 2005 Acta Phys. Sin. 54 5130 (in Chinese) [郭立新, 王运华, 吴振森 2005 物理学报 54 5130]

    [6]

    Ilyushin Y A 2004 Planet. Space Sci. 52 1195

    [7]

    Ye H X, Jin Y Q 2009 Acta Phys. Sin. 58 4579 (in Chinese) [叶红霞, 金亚秋2009 物理学报 58 4579]

    [8]

    Ren X C, Guo L X 2009 Acta Phys. Sin. 58 1627 (in Chinese) [任新成, 郭立新 2009 物理学报 58 1627]

    [9]

    Kobayashi T, Oya H, Ono T 2002 Earth Planets Space 54 982

    [10]

    Fa W Z, Jin Y Q 2010 Sci. China: Earth Sci. 40 473 (in Chinese) [法文哲, 金亚秋 2010 中国科学:地球科学 40 473]

    [11]

    Nouvel J F, Herique A, Kofman W, Safaeinili A 2004 Radio Sci. 39 RS1013

    [12]

    Nouvel J F, Martelat J E, Herique A, Kofman W 2006 Planet. Space Sci. 54 337

    [13]

    Zhang Z F, Hagfors T, Nielsen E, Picardi G, Mesdea A, Plaut J J 2008 J. Geophys. Res. 113 E05004

    [14]

    Zhang Y, Zhang X J, Fang G Y 2012 Acta Phys. Sin. 61 184203 (in Chinese) [张宇, 张晓娟, 方广有 2012 物理学报 61 184203]

    [15]

    Fung A K 1994 Microwave Scattering and Emission Models and Their Applications (London: Artech House) p55

    [16]

    Kirkpatrick S 1983 Science 220 671

    [17]

    Li S Y, Du Z H, Wu M Y, Zhu J, Li S L 2001 Acta Phys. Sin. 50 1260 (in Chinese) [李树有, 都志辉, 吴梦月, 朱静, 李三立2001 物理学报 50 1260]

    [18]

    Yang X P, Zhai H C 2005 Acta Phys. Sin. 54 1578 (in Chinese) [杨晓苹, 翟宏琛 2005 物理学报 54 1578]

    [19]

    Guo L P, Cheng Z X, Han F T, Liu Y, Zhao Z X 2003 Acta Phys. Sin. 52 2842 (in Chinese) [郭立平, 成之绪, 韩甫田, 柳义, 赵志祥 2003 物理学报 52 2842]

    [20]

    Garnero L, Franchois A, Hugonin J P, Pichot C, Joachimowicz N 1991 IEEE Trans. Microw. Theory Tech. 39 1801

  • [1]

    Ilyushin Y A 2007 Planet. Space Sci. 55 100

    [2]

    Kobayashi T, Oya H, Ono T 2002 Earth Planets Space 54 973

    [3]

    Spagnuolo M G, Grings F, Perna P, Franco M, Karszenbaun H, Ramos V A 2011 Planet. Space Sci. 59 1222

    [4]

    Zhang Y Q, Ge D B 2009 Acta Phys. Sin. 58 4573 (in Chinese) [张玉强, 葛德彪 2009物理学报 58 4573]

    [5]

    Guo L X, Wang Y H, Wu Z S 2005 Acta Phys. Sin. 54 5130 (in Chinese) [郭立新, 王运华, 吴振森 2005 物理学报 54 5130]

    [6]

    Ilyushin Y A 2004 Planet. Space Sci. 52 1195

    [7]

    Ye H X, Jin Y Q 2009 Acta Phys. Sin. 58 4579 (in Chinese) [叶红霞, 金亚秋2009 物理学报 58 4579]

    [8]

    Ren X C, Guo L X 2009 Acta Phys. Sin. 58 1627 (in Chinese) [任新成, 郭立新 2009 物理学报 58 1627]

    [9]

    Kobayashi T, Oya H, Ono T 2002 Earth Planets Space 54 982

    [10]

    Fa W Z, Jin Y Q 2010 Sci. China: Earth Sci. 40 473 (in Chinese) [法文哲, 金亚秋 2010 中国科学:地球科学 40 473]

    [11]

    Nouvel J F, Herique A, Kofman W, Safaeinili A 2004 Radio Sci. 39 RS1013

    [12]

    Nouvel J F, Martelat J E, Herique A, Kofman W 2006 Planet. Space Sci. 54 337

    [13]

    Zhang Z F, Hagfors T, Nielsen E, Picardi G, Mesdea A, Plaut J J 2008 J. Geophys. Res. 113 E05004

    [14]

    Zhang Y, Zhang X J, Fang G Y 2012 Acta Phys. Sin. 61 184203 (in Chinese) [张宇, 张晓娟, 方广有 2012 物理学报 61 184203]

    [15]

    Fung A K 1994 Microwave Scattering and Emission Models and Their Applications (London: Artech House) p55

    [16]

    Kirkpatrick S 1983 Science 220 671

    [17]

    Li S Y, Du Z H, Wu M Y, Zhu J, Li S L 2001 Acta Phys. Sin. 50 1260 (in Chinese) [李树有, 都志辉, 吴梦月, 朱静, 李三立2001 物理学报 50 1260]

    [18]

    Yang X P, Zhai H C 2005 Acta Phys. Sin. 54 1578 (in Chinese) [杨晓苹, 翟宏琛 2005 物理学报 54 1578]

    [19]

    Guo L P, Cheng Z X, Han F T, Liu Y, Zhao Z X 2003 Acta Phys. Sin. 52 2842 (in Chinese) [郭立平, 成之绪, 韩甫田, 柳义, 赵志祥 2003 物理学报 52 2842]

    [20]

    Garnero L, Franchois A, Hugonin J P, Pichot C, Joachimowicz N 1991 IEEE Trans. Microw. Theory Tech. 39 1801

计量
  • 文章访问数:  5383
  • PDF下载量:  546
  • 被引次数: 0
出版历程
  • 收稿日期:  2012-08-21
  • 修回日期:  2012-09-06
  • 刊出日期:  2013-02-05

/

返回文章
返回